Small Bodies Near and Far (SBNAF): A benchmark study on physical and thermal properties of small bodies in the Solar System

  title={Small Bodies Near and Far (SBNAF): A benchmark study on physical and thermal properties of small bodies in the Solar System},
  author={Thomas G. Muller and A. Marciniak and Cs. Kiss and Ren{\'e} Duffard and V'ictor Al'i-Lagoa and Przemysław Bartczak and M. Butkiewicz-Bkak and G. Dudzi'nski and Estela Fern'andez-Valenzuela and G{\'a}bor Marton and Nicol{\'a}s Morales and Jos{\'e} Luis Ortiz and Dagmara Oszkiewicz and T Santana-Ros and R'obert Szak'ats and Pablo Santos-Sanz and Andr{\'a}s Farkas and E. Varga-Vereb'elyi},
  journal={Advances in Space Research},
Abstract The combination of visible and thermal data from the ground and astrophysics space missions is key to improving the scientific understanding of near-Earth, main-belt, trojans, centaurs, and trans-Neptunian objects. To get full information on a small sample of selected bodies we combine different methods and techniques: lightcurve inversion, stellar occultations, thermophysical modelling, radiometric methods, radar ranging and adaptive optics imaging. The SBNAF project will derive size… Expand

Figures from this paper

Small Bodies Near and Far (SBNAF): Characterization of asteroids and TNOs
We present results from an EU Horizon2020-funded benchmark study (2016-2019) that addresses critical points in reconstructing physical and thermal properties of near-Earth, main-belt, andExpand
Ground-based Observations of Small Solar System Bodies : Probing Our Local Debris Disk Thematic Areas
Small bodies (comets and asteroids) are a window into the formation, evolution, and dynamic environment of our solar system, an end-state of debris disks that we can only study from afar.Expand
Stellar occultations by Trans-Neptunian objects: From predictions to observations and prospects for the future
Most of the aspects involved in the complex process to successfully observe occultations are reviewed, and some of the lessons learned may allow an increase in the success rate and scientific output of the occultation technique applied to TNOs, in the short-term future. Expand
Stellar Occultations by Transneptunian objects: from Predictions to Observations and Prospects for the Future.
In terms of scientific output, the best way to study solar system bodies is sending spacecraft to make in-situ measurements or to observe at close distance. Probably, the second best means to learnExpand
Small Solar System Bodies as granular media
Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetaryExpand
Database on detected stellar occultations by small outer Solar System objects
Observation of stellar occultation by objects of the Solar System is a powerful technique that allows measurements of size and shape of the small bodies with accuracies in the order of the kilometre.Expand
The AKARI IRC asteroid flux catalogue: updated diameters and albedos
The AKARI IRC All-sky survey provided more than twenty thousand thermal infrared observations of over five thousand asteroids. Diameters and albedos were obtained by fitting an empirically calibratedExpand
Precise astrometry and diameters of asteroids from occultations – a data set of observations and their interpretation
Occultations of stars by asteroids have been observed since 1961, increasing from a very small number to now over 500 annually. We have created and regularly maintain a growing data-set of more thanExpand
Physical parameters of selected Gaia mass asteroids
Thanks to the Gaia mission, it will be possible to determine the masses of approximately hundreds of large main belt asteroids with very good precision. We currently have diameter estimates for allExpand
(704) Interamnia: a transitional object between a dwarf planet and a typical irregular-shaped minor body
Context. With an estimated diameter in the 320–350 km range, (704) Interamnia is the fifth largest main belt asteroid and one of the few bodies that fills the gap in size between the four largestExpand


TNOs are Cool: A Survey of the Transneptunian Region
Over one thousand objects have so far been discovered orbiting beyond Neptune. These trans-Neptunian objects (TNOs) represent the primitive remnants of the planetesimal disk from which the planetsExpand
Asteroids as calibration standards in the thermal infrared for space observatories
Asteroids have been used extensively as calibration sources for the Infrared Space Observatory (ISO) and are planned to be used by future groundbased, airborne and space-based projects in the thermalExpand
(25143) Itokawa : The power of radiometric techniques for the interpretation of remote thermal observations in the light of the Hayabusa rendezvous results (New Insights into Near-Earth and Main-Belt Asteroids)
The near-Earth asteroid (25143) Itokawa was characterized in great detail by the Japanese Hayabusa mission. We revisited the available thermal observations in the light of the true asteroidExpand
3D shape of asteroid (6) Hebe from VLT/SPHERE imaging: Implications for the origin of ordinary H chondrites
Context. The high-angular-resolution capability of the new-generation ground-based adaptive-optics camera SPHERE at ESO VLT allows us to assess, for the very first time, the cratering record ofExpand
“TNOs are Cool”: A survey of the trans-Neptunian region - VI. Herschel/PACS observations and thermal modeling of 19 classical Kuiper belt objects
Trans-Neptunian objects (TNO) represent the leftovers of the formation of the Solar System. Their physical properties provide constraints to the models of formation and evolution of the variousExpand
Uninterrupted optical light curves of main-belt asteroids from the K2 mission
Context. Because the second reaction wheel failed, a new mission was conceived for the otherwise healthy Kepler space telescope. In the course of the K2 mission, the telescope is staring at the planeExpand
Sizes and albedos of Mars-crossing asteroids from WISE/NEOWISE data
Context. Mars-crossing asteroids (MCs) are a dynamically unstable group between the main belt and the near-Earth populations. Characterising the physical properties of a large sample of MCs can helpExpand
Physical properties of the extreme centaur and super-comet candidate 2013 AZ60
We present estimates of the basic physical properties -- including size and albedo -- of the extreme Centaur 2013 AZ60. These properties have been derived from optical and thermal infraredExpand
Spectral and rotational properties of near-Earth asteroid (162173) Ryugu, target of the Hayabusa2 sample return mission
Context. The JAXA Hayabusa2 mission will perform the first ever sample return from a primitive asteroid. The target near-Earth asteroid (162173) Ryugu will be reached in mid-2018 and its samples willExpand
Thermal and shape properties of asteroid (21) Lutetia from Herschel observations around the Rosetta flyby
Prior to and around the Rosetta flyby of (21) Lutetia, the Herschel Space Observatory performed a collaborative observation campaign with its two photometers observing the asteroid in the farExpand